Discovery and physical characterization as the first response to a potential asteroid collision: The case of 2023 DZ2
Marcel M. Popescu, O. V\u{a}duvescu, Julia de Le\'on, C. de la Fuente, Marcos, R. de la Fuente Marcos, M. O. St\u{a}nescu, M. R. Alarcon, M. Serra, Ricart, J. Licandro, D. Berte\c{s}teanu, M. Predatu, L. Curelaru, F. Barwell,, K. Jhass, C. Boldea, A. Aznar Mac\'ias, L. Hudin

TL;DR
This study demonstrates a rapid, multi-method approach to physically and dynamically characterize near-Earth asteroid 2023 DZ2, assessing its impact threat and confirming it will not impact Earth despite its close orbit.
Contribution
The paper introduces a comprehensive, rapid-response methodology combining observational and computational techniques for threat assessment of potential impactors.
Findings
2023 DZ2 has an X-type asteroid spectrum.
It has a rotation period of approximately 6.27 minutes.
It will not impact Earth due to secular near-resonant behavior.
Abstract
Near-Earth asteroids (NEAs) that may evolve into impactors deserve detailed threat assessment studies. Early physical characterization of a would-be impactor may help in optimizing impact mitigation plans. We first detected NEA 2023~DZ on 27--February--2023. After that, it was found to have a Minimum Orbit Intersection Distance (MOID) with Earth of 0.00005~au as well as an unusually high initial probability of becoming a near-term (in 2026) impactor. We aim to perform a rapid but consistent dynamical and physical characterization of 2023~DZ as an example of a key response to mitigate the consequences of a potential impact. We use a multi-pronged approach, drawing from various methods (observational/computational) and techniques (spectroscopy/photometry from multiple instruments), and bringing the data together to perform a rapid and robust threat assessment.} The visible…
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Taxonomy
TopicsAstro and Planetary Science · Geological and Geochemical Analysis · earthquake and tectonic studies
